Oct 2020 Observing Notes
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Mathématiques Et Espace
Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée. -
NEWSLETTER August 2015
NEWSLETTER August 2015 New Horizons at Pluto Credit NASA This space is reserved for promoting member's businesses. You can place an advert here for a donation to the group. Issue 11 August 2015 Page 1 Contents Cover 1 Contents 2 About the cover picture New Horizons 3-7 Thanet Astronomy Group Contact Details 8 Member's Meeting Dates and Times 9 Advertisement (West Bay Cafe) 10 What we did last month 11 Junior Members Page 12 Advertisement (Renaissance Glass) 13 Book Review 14 What's in the sky this month 15-17 Member's Page 18-19 Did You Know ? 20 Junior Astronomers Club (JAC & Gill) 21 Executive Committee Messages 22 Adult Word Search 23 Junior Word Search 24 Member's For Sale and Wanted 25 Issue 11 August 2015 Page 2 About the Cover Picture NEW HORIZONS New Horizons at Pluto Credit NASA New Horizons The Mission The New Horizons mission is the first mission to Pluto and the Kuiper Belt This mission has sent a space craft to the outer reaches of our Solar System to look at the dwarf planet Pluto, and beyond into the Kuiper Belt. The Kuiper Belt is the region of our Solar System beyond the orbit of the planet Neptune, about 30 Astronomical Units (AU) from the Sun and out to about 50 AU. This region contains the minor planet Pluto and its moons Charon, Hydra, Nix and Styx along with many comets, asteroids and many other small objects mostly made of ice. The Kuiper Belt - Credit: NASA Issue 11 August 2015 Page 3 About the Cover Picture NEW HORIZONS An AU or Astronomical Unit is equal to the distance between the Sun and the Earth about 93,000,000 miles or 150,000,000 km. -
Anousheh Ansari
: Fort Worth Astronomical Society (Est. 1949) August 2010 Astronomical League Member At the August Meeting: Special Guest Anousheh Ansari Club Calendar – 2 – 3 Skyportunities Star Party & Club Reports – 5 House Calls by Ophiuchus – 6 Hubble’s Amazing Rescue – 8 Your Most Important Optics -- 9 Stargazers’ Diary – 11 1 Milky Way Over Colorado by Jim Murray August 2010 Sunday Monday Tuesday Wednesday Thursday Friday Saturday 1 2 3 4 5 6 7 Third Qtr Moon Challenge binary star for August: Make use of the New Viking 1 Orbiter 11:59 pm Moon Weekend for Alvan Clark 11 (ADS 11324) (Serpens Cauda) ceases operation better viewing at the 30 years ago Notable carbon star for August: Dark Sky Site Mars : Saturn O V Aquilae 1.9 Conjunction Mercury at greatest Challenge deep-sky object for August: eastern elongation Venus, Mars and Abell 53 (Aquila) Saturn all within a this evening binocular field of First in-flight New Moon view for the first 12 New Moon shuttle repair Neal Armstrong Weekend Weekend days of August. 15 years ago born 80 years ago 8 9 10 11 12 13 14 New Moon Moon at Perigee Double shadow (224,386 miles) transit on Jupiter 3RF Star Party 10:08 pm 1 pm 5:12am High in SSW Museum Star (A.T. @ 5:21 am) Party Venus : Saturn O . 3 of separation Perseid Meteor Watch Party @ 3RF New Moon Magellan enters Fairly consistent show Weekend orbit around Venus of about 60 per hour 20 years ago 15 16 17 18 19 20 21 Algol at Minima 2:45 am - In NE First Qtr Moon Total Solar 1:14 pm Eclipse in 7 years Nearest arc of totality takes in FWAS Grand Island NE St Joseph MO Meeting With Neptune @ Columbia MO Venus at greatest Opposition Anousheh Algol at Minima eastern elongation N of Nashville TN 11:34pm Low In NE 5 am N of Charleston SC Ansari this evening 22 23 24 25 26 27 28 Full Moon Moon at Apogee 2:05 pm (252,518.miles) GATE CODES Smallest of 2010 1 am to the (within 11 hrs of apogee) DARK SKY SITE will be changed st September 1 BE SURE YOU ARE CURRENT WITH DUES to Astroboy’s Day Job Venus : Mars receive new codes O 2 Conjunction 29 31 30 Anousheh Ansari’s Mission Patch at right. -
Lecture 3 Evolution of X-Ray Binaries.Pptx
Evolution of X-ray binaries Rudy Wijnands Anton Pannekoek Institute for Astronomy University of Amsterdam 30 May 2017 Bologna, Italy Evolution of a binary • Many stars are in binary systems • Stellar evolution can be significantly altered due to mass loss and mass transfer • Binary orbit can expand or shrink considerably during the evolution – Conservative or non-conservative mass transfer Conservative mass transfer • Total mass is conserved – Mtotal = m1 + m2 = constant • Total angular moment is conserved – Consider only Jorbit as Jspin<< Jorbit • Then one can proof that • If more massive star transfers mass – dm1/dt < 0 and m1 > m2 – Then P and a decreases until masses become equal for minimum P and a à runaway Roche-lobe mass transfer! – If mass transfer continues, then orbit expands again Non-conservative mass transfer • General case • What happens if either mass or angular moment are not conserved? – Mass is not conserved when • Mass transfer and loss through stellar wind • Very rapid Roche-lobe overflow – Receiving star cannot accrete all mass and mass is loss through L2 point – Angular moment is not conserved when • Magnetic braking through stellar wind – Wind is forced to co-rotate at large distance with the rotation of the star • Gravitational radiation for close compact binaries • E.g., wind from primary escapes system § dm1/dt < 0, and dm2/dt = 0, • General case for mass transfer in circular orbits § With KJ the change in angular moment § Conservative mass transfer: § Stellar wind loss case: Evolution of a binary • Many stars -
CURRICULUM VITAE: Dr Richard Ignace
CURRICULUM VITAE: Dr Richard Ignace Address: Department of Physics & Astronomy Office of Undergraduate Research College of Arts & Sciences Honors College EAST TENNESSEE STATE UNIVERSITY EAST TENNESSEE STATE UNIVERSITY Johnson City, TN 37614 Johnson City, TN 37614 Email: [email protected] [email protected] Web: faculty.etsu.edu/ignace www.etsu.edu/honors/ug research Phone/Fax: (423) 439-6904 / (423) 439-6905 (423) 439-6073 / (423) 439-6080 EDUCATION Ph.D. in Astronomy, University of Wisconsin 1996 M.S. in Physics, University of Wisconsin 1994 M.S. in Astronomy, University of Wisconsin 1993 B.S. in Astronomy, Indiana University 1991 POSITIONS HELD Aug 2016–present, Consultant, Tri-Alpha Energy Jan 2015–present, Director of Undergraduate Research Activities, East Tennessee State University Aug 2013–present, Full Professor: East Tennessee State University Aug 2007–Jul 2013, Associate Professor: East Tennessee State University Aug 2003–Jul 2007, Assistant Professor: East Tennessee State University Sep 2002–Jul 2003, Assistant Scientist: University of Wisconsin Aug 1999–Aug 2002, Visiting Assistant Professor: University of Iowa Nov 1996–Aug 1999, Postdoctoral Research Assistant: University of Glasgow SELECTED PROFESSIONAL ACTIVITIES Involved with service to discipline, institution, and community As Director of Undergraduate Research & Creative Activities, I administrate grant programs and activ- ities that support undergraduate scholarship, plus advocate for undergraduate research. Successful with publishing scholarly articles and competing for grant funding; author of the astron- omy textbook “Astro4U: An Introduction to the Science of the Cosmos,” of the popular astronomy book “Understanding the Universe,” and co-editor of the conference proceedings “The Nature and Evolution of Disks around Hot Stars” Principal organizer for STELLAR POLARIMETRY: FROM BIRTH TO DEATH, Jun 2011; and THE NATURE AND EVOLUTION OF DISKS AROUND HOT STARS, Jul 2004. -
Jet Propulsion Laboratory ANNUAL REPORT Tonight, on the Planet Mars, the United States of America Made History
National Aeronautics and Space Administration 2 0 1 2 Jet Propulsion Laboratory ANNUAL REPORT Tonight, on the planet Mars, the United States of America made history. The successful landing of Curiosity. President Barack Obama Cover: One of the first views from Mars Curiosity shortly after landing, captured by a fish-eye lens on one of the rover’s front hazard-avoid- ance cameras. Inside Cover: The team in mission control erupts in joy when Curiosity’s first picture reaches Earth. This page: Tiny moon Tethys (upper left) dwarfed by Saturn and its rings, as captured by the Cassini spacecraft. 2 Director’s Message Far page: A colorful bow shock in dust clouds sur- 6 Exploring Mars rounding the giant star Contents Zeta Ophiuchi, imaged 16 Planetary Ventures by the Spitzer Space Telescope. 26 The Home Planet 34 Astronomy and Physics 40 Interplanetary Network 46 Science and Technology 52 Public Engagement 58 Achieving Excellence Can it get any better than this? That would have been an excellent question to ask me the night of August 5, 2012. And I know what my answer would have been: It’s hard to imagine how. Of course, the defining moment for JPL in 2012 was the amaz- ing landing of Mars Science Laboratory’s Curiosity rover that Sunday evening. After all the hard work of design and fabrication Director’s Message Director’s and testing, and redesign as the launch slipped by two years, there was nothing to compare to standing in mission control on the arrival evening and watching as the spacecraft executed its incredibly complex landing sequence that ended with the rover safe on the Red Planet’s surface. -
00E the Construction of the Universe Symphony
The basic construction of the Universe Symphony. There are 30 asterisms (Suites) in the Universe Symphony. I divided the asterisms into 15 groups. The asterisms in the same group, lay close to each other. Asterisms!! in Constellation!Stars!Objects nearby 01 The W!!!Cassiopeia!!Segin !!!!!!!Ruchbah !!!!!!!Marj !!!!!!!Schedar !!!!!!!Caph !!!!!!!!!Sailboat Cluster !!!!!!!!!Gamma Cassiopeia Nebula !!!!!!!!!NGC 129 !!!!!!!!!M 103 !!!!!!!!!NGC 637 !!!!!!!!!NGC 654 !!!!!!!!!NGC 659 !!!!!!!!!PacMan Nebula !!!!!!!!!Owl Cluster !!!!!!!!!NGC 663 Asterisms!! in Constellation!Stars!!Objects nearby 02 Northern Fly!!Aries!!!41 Arietis !!!!!!!39 Arietis!!! !!!!!!!35 Arietis !!!!!!!!!!NGC 1056 02 Whale’s Head!!Cetus!! ! Menkar !!!!!!!Lambda Ceti! !!!!!!!Mu Ceti !!!!!!!Xi2 Ceti !!!!!!!Kaffalijidhma !!!!!!!!!!IC 302 !!!!!!!!!!NGC 990 !!!!!!!!!!NGC 1024 !!!!!!!!!!NGC 1026 !!!!!!!!!!NGC 1070 !!!!!!!!!!NGC 1085 !!!!!!!!!!NGC 1107 !!!!!!!!!!NGC 1137 !!!!!!!!!!NGC 1143 !!!!!!!!!!NGC 1144 !!!!!!!!!!NGC 1153 Asterisms!! in Constellation Stars!!Objects nearby 03 Hyades!!!Taurus! Aldebaran !!!!!! Theta 2 Tauri !!!!!! Gamma Tauri !!!!!! Delta 1 Tauri !!!!!! Epsilon Tauri !!!!!!!!!Struve’s Lost Nebula !!!!!!!!!Hind’s Variable Nebula !!!!!!!!!IC 374 03 Kids!!!Auriga! Almaaz !!!!!! Hoedus II !!!!!! Hoedus I !!!!!!!!!The Kite Cluster !!!!!!!!!IC 397 03 Pleiades!! ! Taurus! Pleione (Seven Sisters)!! ! ! Atlas !!!!!! Alcyone !!!!!! Merope !!!!!! Electra !!!!!! Celaeno !!!!!! Taygeta !!!!!! Asterope !!!!!! Maia !!!!!!!!!Maia Nebula !!!!!!!!!Merope Nebula !!!!!!!!!Merope -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Supernova Star Maps
Supernova Star Maps Which Stars in the Night Sky Will Go Su pernova? About the Activity Allow visitors to experience finding stars in the night sky that will eventually go supernova. Topics Covered Observation of stars that will one day go supernova Materials Needed • Copies of this month's Star Map for your visitors- print the Supernova Information Sheet on the back. • (Optional) Telescopes A S A Participants N t i d Activities are appropriate for families Cre with children over the age of 9, the general public, and school groups ages 9 and up. Any number of visitors may participate. Location and Timing This activity is perfect for a star party outdoors and can take a few minutes, up to 20 minutes, depending on the Included in This Packet Page length of the discussion about the Detailed Activity Description 2 questions on the Supernova Helpful Hints 5 Information Sheet. Discussion can start Supernova Information Sheet 6 while it is still light. Star Maps handouts 7 Background Information There is an Excel spreadsheet on the Supernova Star Maps Resource Page that lists all these stars with all their particulars. Search for Supernova Star Maps here: http://nightsky.jpl.nasa.gov/download-search.cfm © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Star Maps: Stars likely to go Supernova! Leader’s Role Participants’ Role (Anticipated) Materials: Star Map with Supernova Information sheet on back Objective: Allow visitors to experience finding stars in the night sky that will eventually go supernova. -
Stars, Constellations, and Dsos [50 Pts]
Reach for the Stars B – KEY Bonus (+1) TRAPPIST-1 Part I: Stars, Constellations, and DSOs [50 pts] 1. Kepler’s SNR 2. Tycho’s SNR 3. M16 (Eagle Nebula) 4. Radiation pressure (wind) from young stars 5. Cas A 6. Extinction (from interstellar dust) 7. 30 Dor 8. [T10] Tarantula Nebula 9. LMC 10. Sgr A* 11. Gravitational interaction with orbiting stars (based on movement over time) 12. M42 (Orion Nebula) 13. [T8] Trapezium 14. (Charles) Messier 15. NGC 7293 (Helix Nebula) –OR– M57 (Ring Nebula) 16. TP-AGB (thermal pulse AGB) 17. Binary system –OR– stellar winds –OR– stellar rotation –OR– magnetic fields 18. Geminga 19. [T4] Jets from pulsar spin poles 20. X-ray 21. NGC 3603 22. Among the most massive & luminous stars known 23. T Tauri 24. FUors (FU Orionis stars) 25. NGC 602 26. Open cluster 27. LMC –AND– SMC 28. Irregular 29. Tidal forces –OR– gravity of MW 30. M1 (Crab Nebula) 31. PWN (pulsar wind nebula) 32. X-ray 33. M17 (Omega Nebula) 34. Omega Nebula –OR– Swan Nebula –OR– Checkmark Nebula –OR– Horseshoe Nebula 35. NGC 6618 36. Zeta Ophiuchi 37. Bow shock (from moving quickly through the ISM) 38. It “wobbles” across the sky (moves perpendicular to overall proper motion) 39. Procyon (α CMi) 40. Mizar –AND– Alcor 41. Mizar 42. Pollux (β Gem) 43. [T5] High rotational velocity 44. Altair (α Aql) –OR– Regulus (α Leo) –OR– Vega (α Lyr) 45. Polaris (α UMi) 46. Precession 47. Binary with observed Doppler shift of spectral lines 48. Beta Cephei variable (β Cep) 49. -
Making the Invisible Visible: a History of the Spitzer Infrared Telescope Facility (1971–2003)/ by Renee M
MAKING THE INVISIBLE A History of the Spitzer Infrared Telescope Facility (1971–2003) MONOGRAPHS IN AEROSPACE HISTORY, NO. 47 Renee M. Rottner MAKING THE INVISIBLE VISIBLE A History of the Spitzer Infrared Telescope Facility (1971–2003) MONOGRAPHS IN AEROSPACE HISTORY, NO. 47 Renee M. Rottner National Aeronautics and Space Administration Office of Communications NASA History Division Washington, DC 20546 NASA SP-2017-4547 Library of Congress Cataloging-in-Publication Data Names: Rottner, Renee M., 1967– Title: Making the invisible visible: a history of the Spitzer Infrared Telescope Facility (1971–2003)/ by Renee M. Rottner. Other titles: History of the Spitzer Infrared Telescope Facility (1971–2003) Description: | Series: Monographs in aerospace history; #47 | Series: NASA SP; 2017-4547 | Includes bibliographical references. Identifiers: LCCN 2012013847 Subjects: LCSH: Spitzer Space Telescope (Spacecraft) | Infrared astronomy. | Orbiting astronomical observatories. | Space telescopes. Classification: LCC QB470 .R68 2012 | DDC 522/.2919—dc23 LC record available at https://lccn.loc.gov/2012013847 ON THE COVER Front: Giant star Zeta Ophiuchi and its effects on the surrounding dust clouds Back (top left to bottom right): Orion, the Whirlpool Galaxy, galaxy NGC 1292, RCW 49 nebula, the center of the Milky Way Galaxy, “yellow balls” in the W33 Star forming region, Helix Nebula, spiral galaxy NGC 2841 This publication is available as a free download at http://www.nasa.gov/ebooks. ISBN 9781626830363 90000 > 9 781626 830363 Contents v Acknowledgments -
Final Report the Goddard High Resolution Spectrograph Scientific
NASA-CR-204980 Final Report The Goddard High Resolution Spectrograph Scientific Support Contract NAS5-32494 December 13, 1993 - December 12, 1996 Computer Sciences Corporation 4061 Powder Mill Road Calverton, MD 20705 GHRS SSC Final Report i Contents List of Acronyms iv I. Introduction II. Summary of Activities 4 1 Project Support - Subtask 1 4 1.1 Proposal Preparation and Tracking ..................... 4 1.2 SMOV and Post-COSTAR Calibration ................... 5 1.3 In-Orbit Performance Papers ........................ 7 1.4 Operations Studies .............................. 7 1.4.1 GHRS Efficiency ........................... 7 1.4.2 GHRS Low-Noise Orbits ....................... 8 1.5 Meetings and Information Distribution ................... 9 1.6 Public Information .............................. 9 1.7 The World Wide Web ............................ 10 1.8 The GHRS Science Symposium ....................... 11 2 Data Analysis Facility - Subtask 2 12 2.1 Facility Management ............................. 12 2.2 GHRS Archive ................................ 13 2.3 GHRS Team Software ............................ 15 2.4 General Software Support .......................... 15 2.5 Data Bases .................................. 16 2.6 Data Reduction and Analysis Assistance .................. 17 3 Extragalactic Imagery- Subtask 3 17 3.1 Analysis of R136 ............................... 17 3.2 Eta Carinae .................................. 19 3.3 Star Clusters in M33 ............................. 19 3.3.1 NGC 595 ............................... 20 3.3,2